Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
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Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.
citing papers explorer
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High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
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The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
Hydrodynamical simulations demonstrate that classical bulges enable bar-driven formation of nuclear stellar disks that bifurcate into pressure-supported nuclear star clusters and rotationally-supported nuclear stellar rings after gas depletion.